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Koss, M.Ricci, ClaudioTreister, Ezequiel.Trakhtenbrot, BennyLamperti, IsabellaOh, KyuseokBerney, SimonSchawinski, KevinBaloković, MislavBaronchelli, LindaCrenshaw, D. Michael[BAT AGN Spectroscopic Survey. I. Spectral Measurements, Derived Quantities, and AGN Demographics.]BAT AGN Spectroscopic Survey. I. Spectral Measurements, Derived Quantities, and AGN Demographics.

Kosec, P.Ricci, ClaudioTreister, Ezequiel.Privon, G. C.Brightman, M.Stern, D.Müller-Sánchez, FranciscoKoss, M.Oh, K.Assef T., RobertoGandhi, P.[Investigating the Evolution of the Dual AGN System ESO 509-IG066.]Investigating the Evolution of the Dual AGN System ESO 509-IG066.

Berney, SimonRicci, ClaudioTreister, Ezequiel.Koss, M.Trakhtenbrot, BennyLamperti, IsabellaSchawinski, Kevin|Baloković, MislavCrenshaw, D. MichaelFischer, TravisGehrels, Neil[BAT AGN spectroscopic survey-II. X-ray emission and high-ionization optical emission lines.]BAT AGN spectroscopic survey-II. X-ray emission and high-ionization optical emission lines.

Oh, KyuseokRicci, ClaudioTreister, Ezequiel.Schawinski, KevinKoss, M.Trakhtenbrot, BennyLamperti, IsabellaMushotzky, RichardVeilleux, SylvainBerney, SimonCrenshaw, D. Michael[BAT AGN Spectroscopic Survey - III : an observed link between AGN Eddington ratio and narrow-emission-line ratios.]BAT AGN Spectroscopic Survey - III : an observed link between AGN Eddington ratio and narrow-emission-line ratios.

Ricci, ClaudioBauer, Franz ErikTreister, EzequielPrivon, G. C.Schawinski, K.Blecha, L.Arevalo, P.Armus, LeeHarrison, F.Ho, L. C.Iwasawa, K.Sanders, David B.Stern, Daniel[Growing supermassive black holes in the late stages of galaxy mergers are heavily obscured.]Growing supermassive black holes in the late stages of galaxy mergers are heavily obscured.

Lansbury, George B.Bauer, Franz Erik.Treister, Ezequiel.Ricci, ClaudioAlexander, D. M.Aird, J. A.Gandhi, P.Stern, Daniel.Koss, M.Lamperti, IsabellaAjello, Marco[The NuSTAR Serendipitous Survey: Hunting for the Most Extreme Obscured AGN at >10 keV]The NuSTAR Serendipitous Survey: Hunting for the Most Extreme Obscured AGN at >10 keV

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